Astrodynamics MCP server: TLE/SGP4, Lambert, access windows, porkchop, B-plane targeting.
Copy the AI prompt to install this server into Claude Code, Cursor, or another agent β or use 1-click editor setup below.
One-click editor setup isnβt available for this listing yet β we donβt have a confirmed install command, and weβd rather show nothing than point your editor at the wrong package or host. Follow the projectβs own setup instructions, linked above.
Inspect callable tools, capabilities, and parameters exposed to AI agents by Astrodynamics MCP.
tle_lookupFetch current TLEs by NORAD ID, name, or group β from CelesTrak (default) or Space-Track.
sgp4_propagatePropagate TLEs across UTC ISO 8601 epochs in TEME / ICRF / GCRS / ITRS / CIRS.
lambert_solveSolve Lambert's problem; multi-rev solutions enumerated; two-impulse Ξv on demand.
access_windowsGround-station / observer access intervals over a window, with AOS / LOS / peak elevation.
time_convertUTC / TAI / TT / TDB / UT1 / GPS / TCB / TCG conversions across ISO / JD / MJD / J2000-seconds / Unix.
frame_transformState-vector transforms across ICRF / ITRS / GCRS / TEME / CIRS / TIRS / IAU body-fixed frames.
A Model Context Protocol server that
gives any MCP-capable LLM client (Claude Code, Cursor, ChatGPT desktop,
custom agents) authoritative astrodynamics tools: TLE/SGP4 propagation,
Lambert solving, ground-station access, time-scale and coordinate-frame
conversions, porkchop scans, B-plane targeting, satellite metadata, and
β with optional extras β full NASA GMAT mission execution ([gmat]),
NASA SPICE / NAIF kernel queries ([spice]), and trajectory visualisation
([viz]).
LLMs reason well about astrodynamics concepts but cannot do the
numerical work β they cannot propagate orbits, solve Lambert problems,
or query SPICE ephemerides. astrodynamics-mcp lets you plug
authoritative tools into any MCP-capable client so the LLM calls vetted
upstream libraries instead of fabricating numbers. Every result carries
explicit units; every tool description tunes against an
Inspect AI eval suite
that measures whether the LLM picks the right tool and binds the right
arguments.
| Tool | What it does | Backed by |
|---|---|---|
tle_lookup | Fetch current TLEs by NORAD ID, name, or group β from CelesTrak (default) or Space-Track. | CelesTrak gp.php API Β· Space-Track β |
sgp4_propagate | Propagate TLEs across UTC ISO 8601 epochs in TEME / ICRF / GCRS / ITRS / CIRS. | sgp4 |
lambert_solve | Solve Lambert's problem; multi-rev solutions enumerated; two-impulse Ξv on demand. | lamberthub |
access_windows | Ground-station / observer access intervals over a window, with AOS / LOS / peak elevation. | skyfield |
time_convert | UTC / TAI / TT / TDB / UT1 / GPS / TCB / TCG conversions across ISO / JD / MJD / J2000-seconds / Unix. | astropy.time |
frame_transform | State-vector transforms across ICRF / ITRS / GCRS / TEME / CIRS / TIRS / IAU body-fixed frames. | astropy.coordinates |
porkchop | (depart Γ arrive) Ξv / C3 grid for interplanetary transfers, ASCII contour, summary or full output. | lamberthub + JPL Horizons |
bplane_target | B-plane element calculation and impulsive targeting for hyperbolic flybys. | in-house, JPL Horizons fed |
satellite_metadata | Physical & provenance metadata (mass, dimensions, COSPAR ID, launch, operator, decay status) for a NORAD ID. | ESA DISCOSweb β |
β Credentialed source. Pass credentials as environment variables for
the stdio transport, or in the session-init _meta block for HTTP β see
Credentials.
A tool called without its credential returns a typed
CredentialRequiredError, never a silent failure.
[gmat] extra)Install the [gmat] extra and have a local NASA GMAT
install, and five more tools register for driving real GMAT missions
(they stay hidden otherwise):
| Tool | What it does | Backed by |
|---|---|---|
gmat_run_mission | Run a complete GMAT mission; returns a parsed summary, report data, and pointers to large outputs. | gmat-run |
gmat_sweep | Parameter sweeps and Monte Carlo (grid / samples / Monte Carlo / Latin hypercube) over a mission. | gmat-sweep |
gmat_execute_script | Escape hatch β run raw GMAT script text and return its reports verbatim; engine errors come back as data. | gmat-run |
gmat_validate_script | Parse-validate a script without running it; returns errors, warnings, and the resource/command structure. | gmat-run |
gmat_read_run_artefact | Read the raw text of a file produced by a prior run (ephemerides, reports too large to inline). | run registry |
[spice] extra)Install the [spice] extra and seven more tools register, backed by NASA
NAIF's CSPICE through spiceypy
(they stay hidden otherwise). They furnish kernels into a process-global
pool and query whatever the pool holds:
| Tool | What it does | Backed by |
|---|---|---|
spice_load_kernel | Furnish a kernel into the pool from a local path or a NAIF https URL (allowlisted, cached); a meta-kernel furnishes all it lists. | spiceypy Β· NAIF |
spice_list_kernels | List the kernels currently furnished in the pool, optionally filtered by category. | spiceypy |
spice_unload_kernel | Drop a furnished kernel by the name spice_load_kernel returned. | spiceypy |
spice_state | Position / velocity of a target relative to an observer at one or more epochs, from furnished SPK kernels. | spiceypy (SPK) |
spice_frame_transform | Rotate a vector between kernel-defined frames β in particular non-Earth body-fixed frames β or return the rotation matrix. | spiceypy (FK / PCK) |
spice_body_parameters | Read a body's radii, GM, and pole / prime-meridian orientation constants from furnished PCK kernels. | spiceypy (PCK) |
spice_time_convert | Convert between the kernel-defined time systems ET / UTC / SCLK using furnished LSK / SCLK kernels. | spiceypy (LSK / SCLK) |
The kernel model, the NAIF furnish-from-URL allowlist, and the process-global pool's trust boundary are covered on the SPICE integration page.
[viz] extra)Install the [viz] extra and four more tools register, backed by
matplotlib (static PNG plots) and the
gmat-czml sibling (CZML export)
β they stay hidden otherwise. Each returns its picture as an attachment
alongside a numeric summary, so a text-only client still gets the answer:
| Tool | What it does | Backed by |
|---|---|---|
plot_ground_track | Render a satellite's sub-satellite ground track as a PNG over a lon/lat graticule, with the latitude / longitude extent inline. | matplotlib |
plot_trajectory | Render an orbit or transfer arc as a 2D or 3D PNG about a central body, with arc length and apsides inline. | matplotlib |
plot_porkchop | Render a porkchop C3 contour as a PNG from a full porkchop grid result β no recompute β with the best cell marked. | matplotlib |
czml_trajectory | Export a trajectory as a CZML document for a Cesium 3D client, returned as an embedded resource. | gmat-czml |
The attachment model β additive PNG ImageContent / CZML EmbeddedResource
beside the structured summary β and which clients render each kind are covered
on the
Visualisation
page.
Full input / output JSON schemas live on the Tool reference page of the docs site.
Install:
Add to your Claude Code MCP settings:
Restart Claude Code. In a chat:
You: Compute the Hohmann Ξv from a 250 km circular LEO to GEO.
(The model calls
lambert_solvewith the Hohmann geometry and answers β 3.91 km/s, citing the tool output β not the LLM's own weights.)
~/.cursor/mcp.json (or workspace-level .cursor/mcp.json):
Restart Cursor. The tools appear under the astrodynamics server group.
See Pick a client in the docs for ChatGPT desktop, a raw Python MCP smoke client, and the Streamable HTTP transport for remote agents.
| Client | Transport | Verified |
|---|---|---|
| Claude Code | stdio | β Yes |
| Cursor | stdio | β Yes |
| ChatGPT desktop | stdio | β³ Expected to work |
Raw Python (mcp SDK) | stdio | β Yes |
| Remote agents | Streamable HTTP | β³ Expected to work |
| LangGraph / AutoGen / CrewAI | any | β³ Expected to work |
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